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researcher

Shigeyuki Sako

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3
ORCID 0000-0002-8792-2205

identity via Semantic Scholar / OpenAlex

most citedResolved 24.5 micron emission from massive young stellar objects

69 citations · 162 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2008★ 69 cited

Resolved 24.5 micron emission from massive young stellar objects

W. J. de Wit, M. G. Hoare, T. Fujiyoshi +8

Massive young stellar objects (MYSO) are surrounded by massive dusty envelopes. Our aim is to establish their density structure on scales of ~1000 AU, i.e. a factor 10 increase in…

astro-ph2008★ 31 cited

A red supergiant nebula at 25 micron: arcsecond scale mass-loss asymmetries of mu Cep

W. J. de Wit, R. D. Oudmaijer, T. Fujiyoshi +8

We present diffraction limited (0.6") 24.5micron Subaru/COMICS images of the red supergiant mu Cep. We report the detection of a circumstellar nebula, that was not detected at shor…

astro-ph2007★ 62 cited

The Asymmetric Thermal Emission of Protoplanetary Disk Surrounding HD 142527 Seen by Subaru/COMICS

Hideaki Fujiwara, Mitsuhiko Honda, Hirokazu Kataza +8

Mid-infrared (MIR) images of the Herbig Ae star HD 142527 were obtained at 18.8 and 24.5 micron with the Subaru/COMICS. Bright extended arc-like emission (outer disk) is recognized…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.